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Laboratory investigation of factors affecting mercury emissions from soils

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Abstract

This study was performed to identify the individual and combined effects of the most important parameters that control mercury (Hg) emissions from soil surfaces: temperature, UV-B exposure, and soil water content. Both soil temperature and UV-B exposure positively affected Hg emissions; however, the increment in Hg emissions was significantly different between wet and dry soils. Mercury emissions from wet soil were more sensitive to an increase in soil temperature than dry soil; however, at constant temperature dry soil emissions were more sensitive than wet soil to changes in UV-B exposure. It was also observed that even after the relative humidity in the soil pores (RHsp) dropped to nearly 0, the Hg emissions were still higher for initially wet soil than for dry soil, suggesting that initially high water content continued to promote Hg reduction mechanisms for an extended period. These results show the interacting effects of soil moisture with other important parameters. At constant water content, Hg emissions increased the most when the soil was exposed to UV-B radiation, followed by UV-A radiation. With UV-C exposure, atmospheric Hg deposition and O3 destruction were simultaneously observed.

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Acknowledgments

This work was supported in part by Kangwon National University (2012) and by Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education, Science and Technology (2009-0066591).

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Correspondence to Young-Ji Han.

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Park, SY., Holsen, T.M., Kim, PR. et al. Laboratory investigation of factors affecting mercury emissions from soils. Environ Earth Sci 72, 2711–2721 (2014). https://doi.org/10.1007/s12665-014-3177-x

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